J/ApJS/199/38ivo://CDS.VizieR/J/ApJS/199/38doi:10.26093/cds/vizier.21990038CDSLimongi M.Chieffi A.2012-08-01T22:43:03Z2012-07-12T15:44:32ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frstellar-evolutionary-modelssupernovaechemical-abundancesWe present a new set of zero metallicity models in the range 13-80M_{sun}_ together to the associated explosive nucleosynthesis. These models are fully homogeneous with the solar metallicity set we published in Limongi & Chieffi (2006ApJ...647..483L) and will be freely available at the Online Repository for the FRANEC Evolutionary Output (ORFEO) Web site. A comparison between these yields and an average star that represents the average behavior of most of the very metal-poor stars in the range -5.0<[Fe/H]<-2.5 confirms previous findings that only a fraction of the elemental [X/Fe] may be fitted by the ejecta of standard core collapse supernovae.2012ApJS..199...38Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/199/38CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/608/405 : Explosive yields of massive star (z=0-z_{Sun}_) (Chieffi+,J/ApJ/611/452 : Evolution of massive stars (El Eid+, 2004)J/A+AS/103/67 : Evolutionary sequences with MC metallicities (de Loore+ 1994)http://www.iasf-roma.inaf.it/orfeo/public_html/ : O.R.F.E.O. home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/199/38https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/199/38http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/199/38https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/199/38https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/199/38http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/199/38GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/199/38/table1Key evolutionary propertiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIMass[13/80] Initial model masssolMassphys.massintPhaseNuclear burning stagephys.atmol.ionStagechartimeNuclear burning lifetimeyrtime.lifetimedouble<Lp>Average photon luminosity; erg/s1e-07Wphys.luminositydouble<Tc>Average central temperatureKphys.temperaturedouble<rhoc>Average central densityg.cm**-3phys.density;stat.meandoubleMcc? Maximum convective core masssolMassphys.massfloatnullableMHeFinal He core masssolMassphys.massfloatMCFinal CO core masssolMassphys.massfloatlogTLog of final effective temperaturelog(K)phys.temperature.effectivefloatlogLLog of final luminositylog(solLum)phys.luminosityfloatJ/ApJS/199/38/table2Explosion properties and ejected masses for all the computed modelsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintParamExplosion property or isotope ejected mass (1)meta.notecharM13Param value in the 13 solar mass modelphys.massdoubleM15Param value in the 15 solar mass modelphys.massdoubleM20Param value in the 20 solar mass modelphys.massdoubleM25Param value in the 25 solar mass modelphys.massdoubleM30Param value in the 30 solar mass modelphys.massdoubleM35Param value in the 35 solar mass modelphys.massdoubleM50Param value in the 50 solar mass modelphys.massdoubleM80Param value in the 80 solar mass modelphys.massdouble